The Expanding Universe: What Does "Creating Space" Really Mean?
Artistic representation of cosmic expansion in which space itself dilates, causing galaxies to move apart.
Image source: astronoo.com (new window), AI-generated image, public domain.
Scientific Abstract
The Astronoo article explores the notion of space creation in an expanding Universe. It explains that cosmic expansion does not correspond to the production of a substance, but to a dynamic evolution of the spacetime metric. Hubble's law, the discovery of cosmic acceleration and the hypothesis of dark energy are presented. The text distinguishes comoving points from the local motion of galaxies, and shows that general relativity describes this dilation through the scale factor. The article finally emphasizes that this phenomenon, though very real, belongs to a geometric interpretation and not to a material creation of vacuum.
Does the Universe really create space as it expands?
This article is devoted to the expansion of the Universe and to the often misunderstood question of "space creation". Since Edwin Hubble's work in 1929, followed by the 1998 discovery of cosmic acceleration, cosmologists have known that distances between distant galaxies increase. But what does this expansion really mean? The answer: it is not the manufacture of a material vacuum, nor a displacement of galaxies within a pre-existing space. What evolves is the geometry of the Universe, that is, the metric that defines distances between points of spacetime. Galaxies retain their comoving position, but the "ruler" that measures their separations changes with time. This dilation is described by the Friedmann-Lemaître-Robertson-Walker metric, within the framework of general relativity. Dark energy, which accounts for about 68% of the Universe's content, is thought to be responsible for the acceleration of this expansion.
Also worth exploring
Continue your exploration of the Universe with these topics:
The Paradox of Space Creation
Hubble's law and the measurement of expansion
In 1929, Edwin Hubble provided the first observational evidence of the expansion of the Universe by establishing the relation between the distance of galaxies and their recession velocity. This relation, known as Hubble's law, is expressed by the formula v = H₀ × d, where v is the recession velocity, d the distance and H₀ the Hubble constant.
Cosmic acceleration and dark energy
In 1998, two independent teams studying type Ia supernovae made a revolutionary discovery: the expansion of the Universe is not slowing down as expected, but is accelerating. This observation, awarded the 2011 Nobel Prize in Physics, implies the existence of a repulsive energy, dubbed "dark energy", which would make up about 68% of the energy content of the Universe.
The table below summarizes the composition of the Universe and the role of each component in the dynamics of expansion.
| Component | Percentage | Effect on expansion | Nature |
|---|---|---|---|
| Dark energy | ~68% | Acceleration | Unknown, negative pressure |
| Dark matter | ~27% | Deceleration | Non-baryonic, gravitational interaction only |
| Ordinary matter | ~5% | Deceleration | Atoms, stars, galaxies |
Does the Expanding Universe "Create Space"?
The concept of comoving points
The concept of "space creation" in the expanding Universe is subtle and often misinterpreted. It is not about the appearance of new space from "nothing" in the philosophical sense, but about the increase of the proper distance between comoving points of spacetime.
N.B.:
Comoving points designate fixed coordinates in the expanding Universe.
A distant galaxy retains its comoving position, even though the distance separating us from it increases with the scale factor.
In other words, it does not "move" locally but follows the expansion of the cosmological metric.
If it is not space, what is "created"?
The dynamic geometry of the Universe
When we say that the Universe "creates space", we must not imagine a manufacture of vacuum, as if the Universe were producing some kind of invisible matter. In reality, what evolves is the geometry of the Universe, that is, the way distances are measured between two points.
"Expansion" concerns the way we measure distances
In physicists' language, the very structure of spacetime is dynamic: the coordinates of distant galaxies remain fixed (they are said to be comoving), but the "ruler" used to measure distances changes over time. It is therefore not a material "fabric" that dilates, but the metric that evolves.
In other words, the Universe does not add volume as one inflates a balloon with air, it recomputes continuously what it means to be separated by a million light-years. What is "created" is neither vacuum nor a mysterious substance, but a relative increase of distances between distant cosmic objects.
A mathematical concept rather than a physical creation of space
Saying that the Universe "creates space" is an imagery way of translating a mathematical reality. In cosmology, one does not manipulate a material fabric but a metric, that is, a formula that indicates how to calculate distances between two points of the Universe. When accelerated expansion is at play, it is this metric that changes with time.
Thus, it is not "space" as a substance that multiplies, but the geometric relation between points that transforms. The Friedmann-Lemaître-Robertson-Walker (FLRW) metric provides the framework: it shows that the scale factor increases, which is equivalent to saying that two comoving galaxies see their distance grow even though they do not move locally.
This vocabulary is useful for popularization, but one must keep in mind that it is a shortcut: what is really described is a dynamic evolution of the geometric equations of general relativity: \( G_{\mu\nu} + \Lambda g_{\mu\nu} = \frac{8 \pi G}{c^4} T_{\mu\nu} \)
Galaxies that "move away"?
An apparent recession, not a local motion
In many illustrations, galaxies are drawn ever farther apart, as if they were really moving through an already existing space. But within the framework of general relativity, that is not how expansion should be understood. Distant galaxies do not "travel" across the cosmos, they keep their position in the comoving grid, while it is this grid, the metric itself, that is measured differently over time. In other words, it is the metric itself that changes scale with time. It is not a substance that deforms, but the rules of measurement (distances, intervals) that stretch.
N.B.:
Very distant galaxies receding at so-called "faster-than-light" speeds do not violate special relativity, because they do not correspond to a local motion but to the evolution of geometry itself.
References
FAQ: Everything you need to know about space creation
Does the Universe really create space?
No, strictly speaking, the Universe does not manufacture space as one would produce a substance. What is called "space creation" refers to the increase of distances between distant galaxies. This dilation results from the evolution of the spacetime metric, described by general relativity. Galaxies do not move within a pre-existing space: it is the geometry of the Universe itself that changes with time.
What is Hubble's law?
Formulated in 1929 by Edwin Hubble, Hubble's law establishes a linear relation between the distance of a galaxy and its recession velocity: the farther a galaxy is, the faster it recedes. It is written v = H₀ × d, where H₀ is the Hubble constant. This law constitutes the first observational evidence of the expansion of the Universe.
What is dark energy?
Dark energy is a hypothetical repulsive form of energy that would make up about 68% of the energy content of the Universe. Discovered indirectly in 1998 through the observation of type Ia supernovae, it is thought to be responsible for the acceleration of cosmic expansion. Its physical nature remains unknown to this day.
Do galaxies recede faster than light?
Some very distant galaxies exhibit an apparent recession velocity greater than that of light. This does not violate special relativity, because it is not a local motion in space, but the expansion of space itself between the galaxies. No signal or object locally crosses this distance at such a speed.
What is a comoving point?
A comoving point is a fixed coordinate in the expanding Universe. A distant galaxy retains its comoving position even if the distance separating us from it increases. This concept makes it possible to distinguish the proper motion of galaxies (negligible on large scales) from the global expansion of the cosmological metric.
Will the expansion of the Universe stop?
Current observations indicate that the expansion of the Universe is accelerating under the effect of dark energy. If this trend continues, the Universe will continue to expand indefinitely, with distant galaxies eventually receding beyond our cosmological horizon. No collapse scenario (Big Crunch) is favored by current data.
Beyond Our Senses: What the Universe Still Hides from Us
Little Red Dots: The Compact Enigmas of the Early Universe
The Weak and Strong Anthropic Principles: Two Ways of Reading the Same Universe
The Universe: Matter... or Information?
Dark Energy: The Most Mysterious Force in the Universe
The Fountains of Creation: The Myth of White Holes
The Great Silence: 10 Insurmountable Walls to Meeting E.T.
Why the Cause Always Precedes the Effect: The Order of the World is Written in This Principle
Absolute Zero and Nothingness: Two Limits the Universe Refuses to Reach
Economical Nature: The Secrets of Conserved Quantities
The Incredible Precision of the Universe's Laws: Chance or Necessity?
The Mystery of the Arrow of Time: Why Can't We Go Back?
The Big Bang: At the Frontiers of the Model
When Space Bends: The Tiny Slope That Guides the Universe
Nabataean Astronomy: Masters of the Desert Between Starry Skies and Stone Constructions
Polynesian Astronomy: The Art of Navigating the Pacific Ocean
Mesopotamian Astronomy: The Cradle of Celestial Observation
Andean Astronomy: A Sacred Link Between Sky and Earth
Ancient Persian Astronomy: Between Babylon and the Islamic Golden Age
Mayan Astronomy: Celestial Cycles Dictated Religious, Agricultural, and Political Time
Islamic Astronomy: When Baghdad Illuminated the Sky of Science
Indian Astronomy: From Sacred Poetry to Scientific Thought
Ancient Greek Astronomy: The Universe of Philosophers in Search of Cosmic Order
The Three Cosmic Shapes: A Hidden Geometry of the Universe
Egyptian Astronomy: Between Sky and Nile, the Secrets of Time
Babylonian Astronomy: When the Sky Predicted Destiny
Chinese Imperial Astronomy: A Millennial Scientific Legacy
Extreme Cosmic Objects: Where Physics Explodes
Mirror Universe: Coexistence of Two Worlds in a Cosmic Reflection
The first second of our history
Time Dilation: Relativistic Mirage or Reality?
Space Through Time: A Constantly Evolving Concept
The Expanding Universe: What Does "Creating Space" Really Mean?
From Nothingness to the Cosmos: Why Is There Something Rather Than Nothing?
How can the Universe measure 93 billion light-years?
How can we say that the Universe has an age?
First Proof of the Expansion of the Universe
Space-time slices of the observable Universe
When the Universe Was Blind: The Long Night Before the First Stars
Alternative theories to the accelerated expansion of the universe
The primitive atom: the first cosmological theory
Great walls and filaments: the great structures of the Universe
The Origins of the Universe: A History of Cosmic Representations
Lyman-alpha Blobs: Gaseous Traces of the First Galaxies
Perspective on the Inflation of the Universe
The Planck Universe: the Image of the Universe Becomes Clearer
The sky is immense with Laniakea
The Symmetries of the Universe: A Journey Between Mathematics and Physical Reality
The Geometry of Time: Exploring the Fourth Dimension of the Universe
How to measure distances in the Universe?
Why ‘nothing’ is impossible: Do nothingness and emptiness exist?
The Horizon Problem: Understanding the Uniformity of the Cosmos
What is Dark Matter? The Invisible Force Shaping the Universe
Metaverse, the next stage of evolution
Multiverse: An Ocean where each Spacetime Bubble has its own Physical Laws
Cosmological Recombination: When the Universe Became Transparent
Cosmological constants: the fine-tuning of the universe
The Thermodynamics of the Sandpile and the Avalanche Effect
The engine of the accelerated expansion of the Universe
The X-Ray Universe: When Space Becomes Transparent
The oldest galaxies in the universe
Hubble constant and expansion of the Universe
Dark Energy: When the Universe Defies Its Own Gravity
What is the Size of the Universe? Between Cosmological Horizon and Infinity
Quantum Vacuum and Virtual Particles: The Physical Reality of Nothingness
Paradox of the dark night
Journey into the Heart of Paradoxes: The Enigmas That Revolutionized Science
Cosmic Microwave Background: The Thermal Echo of the Big Bang